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Fig. F.1

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Posterior distributions for the main jump parameters used in the emcee fit (see Sect. 5): the effective temperature (Teff), the metallicity ([Fe/H]), the log of the stellar density (log ρ*), the log of the stellar mass (log M*), the dilution in the TESS and z′ bands, the epoch (T0), the transit depth (dF), the log of the orbital period (log P) and the cosine of the orbital inclination of the planet (cos i).

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